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Chapter 19 – Formation of the Universe Why do scientists think the universe is expanding?
I. The singularity – The theorized beginning of the universe. A. All particles of matter in the universe was compressed into a unimaginably dense  object  about the size of a dime. B.  Suddenly  this single atom imploded and with a great release of energy all matter began expanding with tremendous speed to create our universe
[object Object],[object Object],[object Object],[object Object],[object Object]
 
B. Inflation Theory 1. For a very short period of time (10 –30 sec) the universe  doubled  itself every 10 –34 sec. 2. This theory was proposed in 1979 by  Alan Guth . 3. This period of great expansion helped establish the law of gravity (All objects have a  gravitational force , the larger the object the greater the force, ex. the earth vs. your pen.) other laws of physics were established between subatomic particles. This theory also helps explain how the force of  gravity began to condense clumps  of matter into objects that would eventually form stars and galaxies.
 
C. Size and organization of our universe. 1. There is no end to the universe, due to the nature of space, it  curves . a. Thought to be  90 billion trillion miles  “across”, this is as far out as we can see. b. At this distance, quasars (star like objects) are observed. Quasars give off more energy than 100’s of galaxies combined, thought to represent the earliest stages of the universe formation
 
2. The universe is composed of around 100 billion galaxies, of which the  Milky Way  (our home) is one. a. Galaxies are composed of  100’s of billions  of stars
 
b. There are  3  general shapes: -  Elliptical : older galaxies, more disc shaped
 
-  Spiral : looks like a pin wheel, Milky Way is one.
 
-  Irregular : least common of the  three .
 
c. Galaxies are rushing away from each other, space is  expanding
3. Formation of heavier elements may be found in supernovae. a. Supernovae occur when  giant stars  (much bigger than our sun) explode and immense energy is released (equal to a trillion hydrogen bombs detonating)
 
b. 10 million  degree  temperatures are adequate to create heavier elements necessary for life (carbon, nitrogen, oxygen, sulfur, and phosphorous).
4. Our galaxy the Milky Way (“milky circle”) is about 100,000 light years  across  and 15,000 light years  long.
 
D. Future of our universe – Scientists are measuring the density (amount of mass per unit of area) of our universe, to predict what will happen. A density unit is called  an omega  is used to refer to the density of our universe. Scientists cannot yet measure dark matter (ex. Black holes, neutrinos).
 
1. Open / Eternal Universe ( The Big Rip) If galaxies continue to move away from each other, eventually all  stars will die  and the universe will  fizzle  out.
 
2. Closed Universe ( Big Crunch ) The  gravitational  attraction between  stars  will  overcome the energy that resulted from the  “ Big Bang”. The galaxies will begin to  come  toward  each other, eventually the universe  would  condense  again into another  singularity.
 
3. Flat / Critical Density-  Momentum will be lost, galaxies will stop moving  from each other, the  universe will  not expand , but not contract.  Momentum  will eventually die  and the stars  will fizzle out.
[object Object],[object Object],[object Object],[object Object],[object Object]
2. Direction of this movement is  measured by  a spectroscope which breaks up white light into individual colors (like a prism).
 
3.  Light, like sound, travels in the form of  waves , light just travels A LOT faster ( 186,000 miles a second ). These waves are  measured  in  wavelength  (different wavelengths of light appear as  different   color s)
 
4. Light waves when  approaching  an object are  shorter  with a  higher  frequency (Just as with sound - ex. train whistle sounds high when approaching you). In light,  blue /violet  are the visible colors with  shorte r wavelength. Therefore objects moving toward the earth and giving off light, have a  blue shift  / color to them when measured with a spectroscope
5. Light waves when moving  away  from an object are  longe r with a  lower  frequency (i.e. train whistle sounds lower when moving away from you) –  red  is the visible color with longer wavelengths. Therefore objects that are moving  away  from earth have a  red shift  when measured with spectroscope
 
6. All  galaxies  observed in the universe have a  red shift , so they are moving  away  from our galaxy. 7. The degree of the  shift  (how blue or red) gives information on the  speed  at which the object is moving
 
B. Detection of  uniformly  distributed  cosmic background radiation  (CBR), left over energy from the  Big Bang , is found in the form of  radio waves . 1% of static on TV is this background radiation from the big bang.
C. Chemical  Composition: The big bang model predicts that the universe is about 75%  hydrogen  and about 25%  helium  with small amounts of heavier elements. This is supported by measurements of observable universe.
[object Object],[object Object]
B. 1929 – Edwin Hubble, hypothesized approximate size of the universe and observed “red shift” of neighboring galaxies
 
C. 1948 – George Gamow, speculated that such a Big Bang explosion would have left behind uniformly distributed  background radiation  throughout the universe
D. 1964 – Arno Penzias and Robert Wilson,  discovered  the background radiation coming from all directions
E. 1970’s – Alan Guth, Inflation Theory   explaining laws of physics and formation of galaxies. F. 1992 – George Smoot, measured temperature fluctuations of space at 2.7 Kelvin, evidence of structure of universe
[object Object],[object Object]
 
B. Particles in the  center  of the cloud,   coalesce (come together) faster and become more  dense , increasing temperature causing nuclear  fusion , gives off heat and light (2 hydrogen atoms fuse and form helium)- this is called a protostar (our sun).  99.9%  of all the mass in our solar system is contained in our  sun.
 
C. In the outer portions of the cloud,  colliding dust grains  begin to stick together until they are big enough to produce their own gravitational field, attracting even more matter, forming  protoplanets .
 
[object Object]
 
2. Outer planets (Jupiter, Saturn, Uranus and Neptune) are far enough from the sun that  gases do not burn off  and they tend to be  very large  planets.
 
3. Asteroid belts are thought to be created from clumps of matter that were  not assimilated  into the protoplanets.
There is an asteroid belt between Mars and Jupiter termed the “main belt”, and another on the outer edge of the solar system called the “Kuiper belt”. The “Oort Cloud” is on the outermost edges of our universe and contains a collection of comet-like objects.
 
D. The forming  protoplanets  of the outer portion of the cloud begin to   swirl around the center (sun). Our solar system formed about  4.5 billion years  ago
 
E. It takes our sun  200 million years  to rotate around the core of the Milky Way galaxy.

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Chapter 19 – formation of the universe

  • 1. Chapter 19 – Formation of the Universe Why do scientists think the universe is expanding?
  • 2. I. The singularity – The theorized beginning of the universe. A. All particles of matter in the universe was compressed into a unimaginably dense object about the size of a dime. B. Suddenly this single atom imploded and with a great release of energy all matter began expanding with tremendous speed to create our universe
  • 3.
  • 4.  
  • 5. B. Inflation Theory 1. For a very short period of time (10 –30 sec) the universe doubled itself every 10 –34 sec. 2. This theory was proposed in 1979 by Alan Guth . 3. This period of great expansion helped establish the law of gravity (All objects have a gravitational force , the larger the object the greater the force, ex. the earth vs. your pen.) other laws of physics were established between subatomic particles. This theory also helps explain how the force of gravity began to condense clumps of matter into objects that would eventually form stars and galaxies.
  • 6.  
  • 7. C. Size and organization of our universe. 1. There is no end to the universe, due to the nature of space, it curves . a. Thought to be 90 billion trillion miles “across”, this is as far out as we can see. b. At this distance, quasars (star like objects) are observed. Quasars give off more energy than 100’s of galaxies combined, thought to represent the earliest stages of the universe formation
  • 8.  
  • 9. 2. The universe is composed of around 100 billion galaxies, of which the Milky Way (our home) is one. a. Galaxies are composed of 100’s of billions of stars
  • 10.  
  • 11. b. There are 3 general shapes: - Elliptical : older galaxies, more disc shaped
  • 12.  
  • 13. - Spiral : looks like a pin wheel, Milky Way is one.
  • 14.  
  • 15. - Irregular : least common of the three .
  • 16.  
  • 17. c. Galaxies are rushing away from each other, space is expanding
  • 18. 3. Formation of heavier elements may be found in supernovae. a. Supernovae occur when giant stars (much bigger than our sun) explode and immense energy is released (equal to a trillion hydrogen bombs detonating)
  • 19.  
  • 20. b. 10 million degree temperatures are adequate to create heavier elements necessary for life (carbon, nitrogen, oxygen, sulfur, and phosphorous).
  • 21. 4. Our galaxy the Milky Way (“milky circle”) is about 100,000 light years across and 15,000 light years long.
  • 22.  
  • 23. D. Future of our universe – Scientists are measuring the density (amount of mass per unit of area) of our universe, to predict what will happen. A density unit is called an omega is used to refer to the density of our universe. Scientists cannot yet measure dark matter (ex. Black holes, neutrinos).
  • 24.  
  • 25. 1. Open / Eternal Universe ( The Big Rip) If galaxies continue to move away from each other, eventually all stars will die and the universe will fizzle out.
  • 26.  
  • 27. 2. Closed Universe ( Big Crunch ) The gravitational attraction between stars will overcome the energy that resulted from the “ Big Bang”. The galaxies will begin to come toward each other, eventually the universe would condense again into another singularity.
  • 28.  
  • 29. 3. Flat / Critical Density- Momentum will be lost, galaxies will stop moving from each other, the universe will not expand , but not contract. Momentum will eventually die and the stars will fizzle out.
  • 30.
  • 31. 2. Direction of this movement is measured by a spectroscope which breaks up white light into individual colors (like a prism).
  • 32.  
  • 33. 3. Light, like sound, travels in the form of waves , light just travels A LOT faster ( 186,000 miles a second ). These waves are measured in wavelength (different wavelengths of light appear as different color s)
  • 34.  
  • 35. 4. Light waves when approaching an object are shorter with a higher frequency (Just as with sound - ex. train whistle sounds high when approaching you). In light, blue /violet are the visible colors with shorte r wavelength. Therefore objects moving toward the earth and giving off light, have a blue shift / color to them when measured with a spectroscope
  • 36. 5. Light waves when moving away from an object are longe r with a lower frequency (i.e. train whistle sounds lower when moving away from you) – red is the visible color with longer wavelengths. Therefore objects that are moving away from earth have a red shift when measured with spectroscope
  • 37.  
  • 38. 6. All galaxies observed in the universe have a red shift , so they are moving away from our galaxy. 7. The degree of the shift (how blue or red) gives information on the speed at which the object is moving
  • 39.  
  • 40. B. Detection of uniformly distributed cosmic background radiation (CBR), left over energy from the Big Bang , is found in the form of radio waves . 1% of static on TV is this background radiation from the big bang.
  • 41. C. Chemical Composition: The big bang model predicts that the universe is about 75% hydrogen and about 25% helium with small amounts of heavier elements. This is supported by measurements of observable universe.
  • 42.
  • 43. B. 1929 – Edwin Hubble, hypothesized approximate size of the universe and observed “red shift” of neighboring galaxies
  • 44.  
  • 45. C. 1948 – George Gamow, speculated that such a Big Bang explosion would have left behind uniformly distributed background radiation throughout the universe
  • 46. D. 1964 – Arno Penzias and Robert Wilson, discovered the background radiation coming from all directions
  • 47. E. 1970’s – Alan Guth, Inflation Theory explaining laws of physics and formation of galaxies. F. 1992 – George Smoot, measured temperature fluctuations of space at 2.7 Kelvin, evidence of structure of universe
  • 48.
  • 49.  
  • 50. B. Particles in the center of the cloud, coalesce (come together) faster and become more dense , increasing temperature causing nuclear fusion , gives off heat and light (2 hydrogen atoms fuse and form helium)- this is called a protostar (our sun). 99.9% of all the mass in our solar system is contained in our sun.
  • 51.  
  • 52. C. In the outer portions of the cloud, colliding dust grains begin to stick together until they are big enough to produce their own gravitational field, attracting even more matter, forming protoplanets .
  • 53.  
  • 54.
  • 55.  
  • 56. 2. Outer planets (Jupiter, Saturn, Uranus and Neptune) are far enough from the sun that gases do not burn off and they tend to be very large planets.
  • 57.  
  • 58. 3. Asteroid belts are thought to be created from clumps of matter that were not assimilated into the protoplanets.
  • 59. There is an asteroid belt between Mars and Jupiter termed the “main belt”, and another on the outer edge of the solar system called the “Kuiper belt”. The “Oort Cloud” is on the outermost edges of our universe and contains a collection of comet-like objects.
  • 60.  
  • 61. D. The forming protoplanets of the outer portion of the cloud begin to swirl around the center (sun). Our solar system formed about 4.5 billion years ago
  • 62.  
  • 63. E. It takes our sun 200 million years to rotate around the core of the Milky Way galaxy.